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Table 3

Initial fractional fractional abundances (f0X$f^{\rm X}_{0}$), effective radii (re) and expansion velocities (Vexp) derived from radiative transfer modelling.

Molecule f0X$f^{\rm X}_{0}$ index re (cm) Vexp km s−1
T Dra (C-rich with X-rays)
HCO+ (2024) 3.0×10−8 3.0×1016 10.0
HCO+ (2020) 1.5×10−8 3.0×1016 10.0
HCN 8.0×10−5 6.0×1015 12.0
HC3N 1.2×10−5 1.7×1015 10.0
SiO 2.5×10−6 1.8×1015 10.0
SiC2(*) 1.3×10−6 3.0×1016 10.0
C2H(*) 5.0×10−7 1.0×1017 10.0
SiS (*) 2.0×10−7 5.0×1015 8.0
HNC 1.8×10−7 5.0×1015 9.0
N2H+ (*) <3.0× 10−8 1.0×1016 10.0
EY Hya (O-rich with X-rays)
HCO+ (*) <1.0×10−7 1.0×1016 6.0
SiO 2.0×10−7 1.0×1016 6.0
VY Uma (C-rich without X-rays)
HCO+ (*) <5.0×10−8 1.0×1016 5.5
HCN 1.5×10−6 8.0×1014 5.5
V Eri (O-rich without X-rays)
HCO+ (*) <3.0×10−8 1.0×1016 6.0
SiO 2.0×10−7 7.0×1015 6.0

Notes. Column (1): molecule, Col. (2): initial abundance relative to H2, Col (3): effective radius, Col (4): expansion velocity. (*) Indicates that re and Vexp were assumed (see Sect. 5.3).

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